日本地球惑星科学連合2014年大会

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インターナショナルセッション(口頭発表)

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM06_1AM1] Study of coupling processes in Sun-Earth system with large radars and large-area observations

2014年5月1日(木) 09:00 〜 10:45 312 (3F)

コンビーナ:*山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学太陽地球環境研究所)、橋口 浩之(京都大学生存圏研究所)、座長:小川 泰信(国立極地研究所)

10:15 〜 10:30

[PEM06-21] FPIとISレーダーで観測された脈動オーロラ中の熱圏風速変動

*大山 伸一郎1栗原 純一2津田 卓雄3塩川 和夫1三好 由純1ワトキンス ブレントン J.4 (1.名古屋大学太陽地球環境研究所、2.北海道大学大学院理学研究院、3.国立極地研究所、4.Geophysical Institute, University of Alaska Fairbanks)

キーワード:脈動オーロラ, 熱圏, FPI, ISレーダー

Pulsating aurora is a typical phenomenon of the recovery phase of magnetic substorm and is frequently observed in the morning sector. While our understanding of pulsating aurora has not yet reached maturity, the widely accepted generation mechanism causing pulsations in precipitating electrons is related to wave-particle interactions around the equatorial plane in the magnetospheric tail. The closure current system in pulsating aurora may not be as strongly evolved as compared to that in the discrete arc because of smaller precipitation flux (or upward field-aligned current) and weaker perpendicular electric field (or the Pedersen current). Thus one may assume that Joule energy dissipation and/or Lorentz force does not play an important role for modifications of the thermospheric wind dynamics in pulsating aurora. However, we found thermospheric-wind variations in the pulsating aurora during simultaneous observations with a Fabry-Perot Interferometer (FPI; 557.7 nm), an all-sky camera (557.7 nm), and the European Incoherent Scatter (EISCAT) UHF radar. Of particular interest is that the location of the fluctuations was found in a darker area that appeared within the pulsating aurora. During the same time period, the EISCAT radar observed sporadic enhancements in the F-region backscatter echo power, which suggests the presence of low-energy electron (1 keV or lower) precipitation. Using other data sets archived by the EISCAT radar, a statistical analysis shows that the F-region enhancement tends to coexist with hard-particle precipitation or the pulsating aurora. This presentation will summarize our experimental evidences showing several events of the pulsating aurora, and discuss application of the phased-array IS radar to this study.